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Evolution of Planetary Chaotic Zones in Planetesimal Disks. / Demidova, T. V.; Shevchenko, I. I.

в: Astronomy Letters, Том 47, № 11, 11.2021, стр. 771-781.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Demidova, TV & Shevchenko, II 2021, 'Evolution of Planetary Chaotic Zones in Planetesimal Disks', Astronomy Letters, Том. 47, № 11, стр. 771-781. https://doi.org/10.1134/S1063773721110013

APA

Demidova, T. V., & Shevchenko, I. I. (2021). Evolution of Planetary Chaotic Zones in Planetesimal Disks. Astronomy Letters, 47(11), 771-781. https://doi.org/10.1134/S1063773721110013

Vancouver

Demidova TV, Shevchenko II. Evolution of Planetary Chaotic Zones in Planetesimal Disks. Astronomy Letters. 2021 Нояб.;47(11):771-781. https://doi.org/10.1134/S1063773721110013

Author

Demidova, T. V. ; Shevchenko, I. I. / Evolution of Planetary Chaotic Zones in Planetesimal Disks. в: Astronomy Letters. 2021 ; Том 47, № 11. стр. 771-781.

BibTeX

@article{91e830c80c844782adcc47147a63b6d5,
title = "Evolution of Planetary Chaotic Zones in Planetesimal Disks",
abstract = "Abstract: Extensive numerical experiments on the long-term dynamics of planetesimal disks with planets in systems of single stars have been carried out. The planetary chaotic zone clearing timescales (Formula presented.) as a function of mass parameter (Formula presented.) (planet–star mass ratio) have been determined numerically with a high accuracy separately for the outer and inner parts of the chaotic zone. Diffusional components (Formula presented.) have been revealed in the dependence (Formula presented.). The results obtained are discussed and interpreted in light of existing analytical theories based on the mean motion resonance overlap criterion and in comparison with previous numerical approaches to the problem.",
keywords = "debris disks, dynamical chaos, planetary chaotic zones, planetesimal disks, planetesimals",
author = "Demidova, {T. V.} and Shevchenko, {I. I.}",
note = "Publisher Copyright: {\textcopyright} 2021, Pleiades Publishing, Inc.",
year = "2021",
month = nov,
doi = "10.1134/S1063773721110013",
language = "English",
volume = "47",
pages = "771--781",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "11",

}

RIS

TY - JOUR

T1 - Evolution of Planetary Chaotic Zones in Planetesimal Disks

AU - Demidova, T. V.

AU - Shevchenko, I. I.

N1 - Publisher Copyright: © 2021, Pleiades Publishing, Inc.

PY - 2021/11

Y1 - 2021/11

N2 - Abstract: Extensive numerical experiments on the long-term dynamics of planetesimal disks with planets in systems of single stars have been carried out. The planetary chaotic zone clearing timescales (Formula presented.) as a function of mass parameter (Formula presented.) (planet–star mass ratio) have been determined numerically with a high accuracy separately for the outer and inner parts of the chaotic zone. Diffusional components (Formula presented.) have been revealed in the dependence (Formula presented.). The results obtained are discussed and interpreted in light of existing analytical theories based on the mean motion resonance overlap criterion and in comparison with previous numerical approaches to the problem.

AB - Abstract: Extensive numerical experiments on the long-term dynamics of planetesimal disks with planets in systems of single stars have been carried out. The planetary chaotic zone clearing timescales (Formula presented.) as a function of mass parameter (Formula presented.) (planet–star mass ratio) have been determined numerically with a high accuracy separately for the outer and inner parts of the chaotic zone. Diffusional components (Formula presented.) have been revealed in the dependence (Formula presented.). The results obtained are discussed and interpreted in light of existing analytical theories based on the mean motion resonance overlap criterion and in comparison with previous numerical approaches to the problem.

KW - debris disks

KW - dynamical chaos

KW - planetary chaotic zones

KW - planetesimal disks

KW - planetesimals

UR - http://www.scopus.com/inward/record.url?scp=85126212573&partnerID=8YFLogxK

U2 - 10.1134/S1063773721110013

DO - 10.1134/S1063773721110013

M3 - Article

AN - SCOPUS:85126212573

VL - 47

SP - 771

EP - 781

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 11

ER -

ID: 93900405